UVCS MISSION LOG ---------------- Date: 28 September 2007 ----- Last revision: 01 October 2007 (MU) -------------- File Name: 2007.09.29.a.log ---------- Compiled by: M. Uzzo, R. Wu ------------ UVCS Activity: North Polar Coronal Hole LYA Observation for -------------- 29 - 30 September 2007 Load Equatorial Coronal Hole LYA Observation for October 01 2007 Load Equatorial Coronal Hole LYA Observation for October 01 2007 Load Equatorial Coronal Hole LYA Observation for October 01 2007 Load Equatorial Coronal Hole OVI Observation for October 01 2007 Load Equatorial Coronal Hole OVI Observation for October 01 2007 Load Equatorial Coronal Hole OVI Observation for October 01 - 02 2007 SOHO Activity: -------------- EOF Staff: S. Cranmer: Lead Scientist ---------- R. Wu: Commander M. Uzzo: Planner Y.-K. Ko Command file: 07.09.28.11:49:03.cmd.log Activity: --------- 1) North Polar Coronal Hole LYA Observations Sequence: 06.08_hole.tcl, n = 1, m = 1, p = 0, r = 0, e = 2 SCI_SPEC: Characterization of a polar coronal hole. Goal is to measure the properties of a polar coronal hole. In particular we are interested in the coronal conditions (intensities and line widths for HI Ly-alpha and OVI 1032/1037) as a function of height and latitude. We will compare these properties with the ones found in non-polar coronal holes. Roll positions are VL-corrected for PA=0 degrees. OBS_PROG: Primary: Sensitivity Sub Obj: Spatial Coverage SCI_OBJ: Plasma Properties...Proton and Ion Temperatures OBJ: Coronal Hole CMP_NAME: CMP_NUM: Duration: start: 2007.09.29.20:42 end: 2007.09.30.00:13 ONUMs = 23713 (102 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: 353.267 Degrees (17536) - Mirror/Occulter: 2.0 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 50 um - LYA GRTPOS: 100000 - OVI GRTPOS: 164600 - OVI MCP Voltage: 200 - OVI mask: OVI_sp2_164 in slot 4 Fits Files: q07.09.29.20:42:28.ovi.dat